A Python package to interpret the oscillation spectrum of γ Doradus and Slowly Pulsating B stars.
γ Doradus and SPB stars pulsate in low-frequency gravito-inertial modes that carry information about their internal structure and rotation profile. This package allows you to perform mode identification, measure the mean rotation rate and buoyancy radius of these pulsators from a list of frequencies extracted from the oscillation spectrum. morse has been primarily designed to deal with moderately and fastly rotating pulsators but, to some extent, is also of interest for slowly rotating stars.
Documentation: https://morse-asteroseismo.rtfd.io
If you make use of this code for your research, please cite Christophe et al. 2018 (2018, A&A, 618A, 47C).